六頻道光度計之氣輝地面觀測

以作者查詢圖書館館藏

、以作者查詢臺灣博碩士

、以作者查詢全國書目

、勘誤回報

、線上人數：4

、訪客IP：3.145.88.130

姓名

吳欣駿(Shin-Chun Wu) 查詢紙本館藏

畢業系所

物理學系

論文名稱

六頻道光度計之氣輝地面觀測

相關論文

★ 氧氣在105-190nm間高激發態之光譜研究	★ H2O光解產生OH(A2Σ+)振動態之研究
★ 氮氣光譜之研究Ⅰ:C3Πu-X1Σg+及a1Πg- X1Σg+系統	★ 丙炔與丙二烯吸收光譜之研究
★ O2(b1Sg+)氣輝的全球分布與變化	★ 以雷射雷達量測對流層頂之溫度、高度分布 -與無線電探空儀量測資料之比較、分析
★ 氮氣光譜之研究Ⅱ: C3Πu-X1Σg+及a1Πg- X1Σg+系統	★ 一氧化氮激態的消光及螢光激發光譜之研究
★ 一氧化氮激態D2Σ+螢光之消激研究	★ 一氧化氮激態A2Σ+螢光之消激研究
★ 中壢上空10–30公里間的卷雲、氣膠、溫度的測量與光散射性質之研究	★ 低對流層氣膠之光達量測
★ 對流層氣膠光學性質之研究	★ 氮氣分子在45-100 nm之光吸收、光離子化、光解離
★ 利用光達技術探測氣膠與水汽之作用	★ 利用地面與空載光達進行熱帶高空卷雲之研究

檔案

[Endnote RIS 格式]

[Bibtex 格式]

[相關文章]

[文章引用]

[完整記錄]

[館藏目錄]

[檢視]

[下載]

本電子論文使用權限為同意立即開放。
已達開放權限電子全文僅授權使用者為學術研究之目的，進行個人非營利性質之檢索、閱讀、列印。
請遵守中華民國著作權法之相關規定，切勿任意重製、散佈、改作、轉貼、播送，以免觸法。

摘要(中)

本論文討論利用六頻道光度計配合10公分Cassegrain望遠鏡進行地面氣輝觀測。六個濾鏡分別為全黑、532 nm、557.7nm、560 nm、589 nm、630 nm，其中全黑頻道用來檢驗儀器的暗電流而557.7nm頻道觀測OI (1S - 1D)氣輝，630 nm頻道觀測OI(1D - 3P )氣輝，589 nm頻道觀測Na (2P - 2S)氣輝，而560 nm頻道用來觀測OH氣輝以及作為557.7nm和589 nm的校正檢驗，另外532 nm頻道為配合532 nm綠光雷射作為雲探測器。數據取樣時間在2013年八月到十月。地點為台灣嘉義鹿林天文台(120° 52′ 25" E 23° 28′ 07" N)，將觀測數據與國家通訊委員會上Ionosonde電離層電子密度數據做比較並討論氣輝強度變化的原因。實驗結果知道電離層內的電子密度與630 nm氣輝強度比較有相關存在且與557.7 nm氣輝強度無關係，利用氣輝與電子探測時間差異估出電離層內擾動變化的分量速度及波長。及589 nm氣輝強度與SABER上氧原子數量變化有相同的變化趨勢。

摘要(英)

An airglow photometer combined with a 10cm telescope is install at the NCU for airglow study. The photometer include six different interference filters to measure the airglow emissions including OI (1S - 1D) 557.7 nm and OI (1D - 3P) 630.0 nm and Na (2P - 2S) 589.0 nm produced in the upper atmospheric. A 560 nm filter is used to measure the background emissions like OH airglow. Another channel at 532 nm is used to measure the background as well as cloud disturbance by measuring the backward scattering signals from a 532 nm laser which is sending into the sky from the observation site. In Aug- Oct., 2013, airglow data has been measured at Lulin observatory (120° 52′ 25" E 23° 28′07" N). The data is compared with Ionosonde measurements to find the correlation between electron content and of airglow intensity. The correlations among different wavelengths are discussed although complex correlation has been observed.

關鍵字(中)

★ 630nm氣輝
★ 557.7nm氣輝

關鍵字(英)

★ 630nm airglow
★ 557.7nm airglow

論文目次

1. 簡介 ................................................................. 1
1.1 歷史介紹 ....................................................... 1
1.2 大氣層與電離層: ................................................ 4
1.3 原子能階: ...................................................... 6
1.3.1 氧原子能階 ............................................... 7
1.3.2 鈉原子能階 ............................................... 7
1.4 反應機制 ....................................................... 9
1.4.1 630 nm OI 紅線 ............................................ 9
1.4.2 557.7nm OI 綠線: ........................................ 10
1.4.3 589 nm 鈉原子黃線: ...................................... 11
1.4.4 OH 氣輝 .................................................. 11
1.5 氣輝變化: ..................................................... 12
1.5.1. 短期變化: ............................................... 13
1.5.1. 長期變化 ................................................ 18
2. 實驗裝置與方法: ..................................................... 21
2.1 實驗儀器: ..................................................... 21
2.2 實驗方法: ................................................... 25
3. 數據分析 ............................................................ 27
3.2 電離層擾動波速分析討論 ........................................ 32
3.3 560/557.7/589 nm 氣輝比較 ..................................... 38
3.4 589 nm 氣輝與 560 nm 氣輝: ...................................... 47
4. 結論 ................................................................ 50
5. 參考文獻 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .54

參考文獻

1. L. Yntema, 1909. On the Brightness of the sky and total amount of strarlight, Publ. Ast. Groningen, vol. 22, pp. 1-55.
2. S. Newcomb, 1901. A Rude Attempt to Determine the Total Light of all the Stars, Astrophys. J., vol. 14, pp. 297.
3. G. J. Burns, 1902. The total light of all the stars, Astrophys. J. vol.16, pp. 166.
4. S. D. Townley, 1902. Planetary Phenomena for March and April, Publ. Ast. Soc. Pacif., vol. 15, pp. 13.
5. J. S. Bowen, 1928. The origin of the nebular lines and the structure of the planetary nebulae. Astrophys. J., vol. 67, pp. 1.
6. I. C. Mcdade, 1997. Laboratory Measurements Required for Upper Atmospheric Remote Sensing of Atomic Oxygen, Advances in Space Research, vol. 19, pp. 653-661.
7. Kelley M.C, 1989. The Earth’s Ionosphere: Electrodynamics and Plasma Physics, Academic Press, Inc., New York.
8. B.G. Fejer et al, 1981. F region East-West Drifts at JICAMARCA.
9. T. F. Malone, 1951. Night Sky Radiations from the Upper AtmosphereCompendiumof Meterology.
10. S. K. Mitra, 1953. The Upper Atmosphere (2nd ed), Calcutta: The Asiatic Society.
11. K. Shiokawa et al, 2003. Statistical study of nighttime medium-scale traveling ionospheric disturbances using mid latitude airglow images. Journal of Geophysical Research, vol. 108, no. A1, pp. 105.
12. T. Ogawa et al, 2002. Observations and modeling of 630 nm airglow and total electron content associated with traveling ionospheric disturbances over Shigaraki, Japan, Earth Planets Space, vol. 54, pp. 45-56.
13. M. Mendillo, A. Tyler ,1983. Geometry of Depleted Plasma Regions in the Equatorial Ionosphere, Journal of Geophysical Research, vol. 88, no. A7, pp. 5778-5782.
14. S. P. Zhang ,G. G. Shepherd, 1999. The influence of the diurnal tide on the O(1S) and OH emission rates observed by WINDII on UARS, Geophysical Research Letters, vol. 26, no. 4, pp. 529-532.
15. L. L. Cogger, V. B. Wickwar, H. C. Carlson, 1974. Combined Airglow and Incoherent Scatter Observations as a Technique for Studying Neutral Atmospheric Variations, Radio Science, vol. 9, no. 2, pp. 205-210.
16. T.N Davis, L.L Smith, 1965. Latitudinal and Seasonal Variations in the Night Airglow, Journal of Geophysical Research, vol. 70, no. 5.
17. H. Takahashi et al, 1998. Dynamical Influence on the Equatorial Airglow Observed from the South American Sector, Advances in Space Research, vol. 21, no. 6, pp. 817~825.
18. S. P. Zhang, G. G. Shepherd, 2008. Variations of the O (1D) and O (1S) peak volume emission rates without direct solar effects, Advances in Space Research, vol. 42, pp. 939-946.
19. J. J. Makela, 2006.A Review of Imaging Low-Latitude Ionospheric Irregularity Processes, Journal of Atmospheric and Solar-Terrestrial Physics, vol. 68, no. 14, pp. 41.
20. J. K. Chung et al, 2007. Enhancement of OI 630.0nm emission at mid-latitudes during an intense magnetic storm, Journal of Atmospheric and Solar-Terrestrial Physics, vol. 69, page. 697-706.
21. A.K. Smith, D. R. Marsh, M. G. Mlynczak and J. C. Mast 2010, Temporal variations of atomic oxygen in the upper mesosphere from SABER, J. Geophys. Res., 115, D18309.

指導教授

倪簡白(Jan-Bai Nee)

審核日期

2014-8-15

推文